Structure of the Spiral Galaxy NGC 300

In 1963, Toomre built up classes of mass models for the highly flattened galaxies which have free parameters n, an and Cn. In order to keep the universal dimension, we adopt parameters bn(Cn2 = an2n+2*bn2/(n-1)!) instead of Cn. Series of the normalized Toomre's mass models (G = Vmax = Rmax = 1,...

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Main Authors: Myung-Hyun Rhee, Mun-Suk Chun
Format: Article
Language:English
Published: Korean Space Science Society (KSSS) 1992-06-01
Series:Journal of Astronomy and Space Sciences
Online Access:http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/1992/v9n1/OJOOBS_1992_v9n1_11.pdf
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spelling doaj-4830731e513e499ea163e839a19532ff2020-11-24T23:23:19ZengKorean Space Science Society (KSSS)Journal of Astronomy and Space Sciences2093-55872093-14091992-06-01911129Structure of the Spiral Galaxy NGC 300Myung-Hyun Rhee0Mun-Suk Chun1Department of Astronomy and Atmospheric Science, Yonsei University, Seoul 120-749, KoreaDepartment of Astronomy and Atmospheric Science, Yonsei University, Seoul 120-749, KoreaIn 1963, Toomre built up classes of mass models for the highly flattened galaxies which have free parameters n, an and Cn. In order to keep the universal dimension, we adopt parameters bn(Cn2 = an2n+2*bn2/(n-1)!) instead of Cn. Series of the normalized Toomre's mass models (G = Vmax = Rmax = 1, n =1 to 7) are derived and the normalized parameters an and bn to an(=an*rmax) and bn(=bn*Vmax/rmax), we can get the generalization of Toomre's mass model.http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/1992/v9n1/OJOOBS_1992_v9n1_11.pdf
collection DOAJ
language English
format Article
sources DOAJ
author Myung-Hyun Rhee
Mun-Suk Chun
spellingShingle Myung-Hyun Rhee
Mun-Suk Chun
Structure of the Spiral Galaxy NGC 300
Journal of Astronomy and Space Sciences
author_facet Myung-Hyun Rhee
Mun-Suk Chun
author_sort Myung-Hyun Rhee
title Structure of the Spiral Galaxy NGC 300
title_short Structure of the Spiral Galaxy NGC 300
title_full Structure of the Spiral Galaxy NGC 300
title_fullStr Structure of the Spiral Galaxy NGC 300
title_full_unstemmed Structure of the Spiral Galaxy NGC 300
title_sort structure of the spiral galaxy ngc 300
publisher Korean Space Science Society (KSSS)
series Journal of Astronomy and Space Sciences
issn 2093-5587
2093-1409
publishDate 1992-06-01
description In 1963, Toomre built up classes of mass models for the highly flattened galaxies which have free parameters n, an and Cn. In order to keep the universal dimension, we adopt parameters bn(Cn2 = an2n+2*bn2/(n-1)!) instead of Cn. Series of the normalized Toomre's mass models (G = Vmax = Rmax = 1, n =1 to 7) are derived and the normalized parameters an and bn to an(=an*rmax) and bn(=bn*Vmax/rmax), we can get the generalization of Toomre's mass model.
url http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/1992/v9n1/OJOOBS_1992_v9n1_11.pdf
work_keys_str_mv AT myunghyunrhee structureofthespiralgalaxyngc300
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